2026-09-28 / UCAC4 525-047565 / (1212) Francette
| # | OBS | Observer | Occ | Meth. | Instr. | CC | TSRC | UT1 | UT2 | UT3 | UT4 | UT2E | UT3E | Dur. | Chrd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | show | Tim Haymes | O+ | VID | M280 | GB | GPS | 03:08:00 | 03:09:10.1 | 03:09:12.93 | 03:10:00 | 0.200 | 0.150 | 2.83 | 87.7 |
| 2 | show | Nikolai Wuensche | O+ | VID | M300 | DE | GPS | 03:08:00 | 03:09:28.46 | 03:09:29.75 | 03:11:00 | 0.050 | 0.050 | 1.29 | 40.0 |
| 3 | show | Konrad Guhl | O+ | CCD | M306 | DE | GPS | 03:07:05 | 03:09:27.82 | 03:09:30.62 | 03:11:41 | 0.040 | 0.050 | 2.80 | 86.8 |
3 observations found in db: sodis
Available (probably) matching predictions (click on the link to switch):| JPL75 : f94d7d80-d9b1-11f1-43f3-c05affff67a9 [db: observed] |
Using prediction f94d7d80-d9b1-11f1-43f3-c05affff67a9 for map and profile fit
| Ellipse and circular profile fits to the timings (chords) |
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Auto-Fit Result: Size = 95 x 88 km a',b' = 47.3, 43.9 km X0,Y0 = -839.4, 35.2 km Mean diameter = 91 km From 3 chords (CCD,VID) You can enter space separated chord numbers (example: 11 4 8) or a method like VIS to ignore all visual timings, or a time source like RAD and NTP (but not GPS). If the plot disappears, then there are less than 2 chords left (too much ignored, go back with browser). Check SiMDA for size and mass data. Check Johnston Archive for satellites. |
| Map with groundtrack and observer stations |
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| Event Details |
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Occultation UUID [and DB] : f94d7d80-d9b1-11f1-43f3-c05affff67a9 [observed] Occultation Date + Time : 2026-09-28 at 03:11:42 UT +/- 0.01 min [1] Object Designation : (1212) Francette Orbit Class : MBA Star Designation : GDR3 0655315973901714688 Star Coordinates (ICRF) : RA = 08 16 26.6753, DE = +14 59 42.502 [2] Star Magnitudes : G = 11.88 mag, RP = 11.17 mag, BP = 12.44 mag Object Magnitude : V = 15.84 mag Estimated Magnitude Drop : 4.0 mag Estimated Max. Duration : 2.7 sec Object Mean Diameter : 82.1 km (src: astorb) Speed of the shadow : 31.0 km/s Elongation to Moon & Sun : 100° (sunlit = 97%), Sun = 62° Cross-track uncertainty : 0.3 mas = 0 km = 0.01 path-width (1-sig) RUWE and duplicate source : 1.0 mas, dup.src = 0 (0:false, 1:true) Ephemeris Reference : JPL75 Note : FP:true [1] time t0 of closest geocentric approach c/a, [2] including proper motion until t0 |
| More Data and Informations |
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